SPECT3D Synthetic Self-Emission X-Ray Imaging of CESZAR Gas-Puff Z-Pinch FLASH Simulations
POSTER
Abstract
We present SPECT3D synthetic x-ray images of the CESZAR gas-puff z-pinch simulations generated with FLASH. SPECT3D is a multi-dimensional, collisional, radiative code developed by Prism, Inc. that computes post-process diagnostic signatures and spectroscopy from the output of radiation hydrodynamics calculations. SPECT3D can natively process output simulation data from FLASH, the high-performance computing, finite-volume radiation magnetohydrodynamics (MHD) code developed by the Flash Center for Computational Science. FLASH has extended physics capabilities that enable the code to treat a broad range of physical processes in astrophysics, laboratory plasma physics, and high energy density physics (HEDP). Recent algorithmic extensions in FLASH have now also enabled the code to directly model Z-pinch experiments. We aim to use SPECT3D to validate FLASH by analyzing and comparing synthetic x-ray images of FLASH simulations to CESZAR gas-puff z-pinch experimental data.
*The Flash Center for Computational Science acknowledges support by the U.S DOE NNSA under Awards DE-NA0003856 and DE-NA0003842, and Subcontracts 536203 and 630138 with LANL and B632670 with LLNL. Support from the U.S. DOE ARPA-E under Award DE-AR0001272 and U.S. DOE Office of Science, Fusion Energy Sciences under Award DE-SC0021990 is also acknowledged.
Presenters
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Mary R McMullan
- University of Rochester